Hubble's constant is probably a little larger than the inverse of the age of the Universe. The reason they are close is somewhat of a coincidence, for example in the standard Lambda-CDM model of the Universe, in the far future the age of the Universe will become vastly larger than the inverse of the Hubble constant, because H asymptotically approaches a constant value.
The dynamics of the standard dark energy models, in which over time the accelerated expansion caused by dark energy dominates, but the expansion in the early Universe was decelerating due to the domination of radiation and then matter, means that at some point the inverse of the Hubble constant must equal the age of the Universe. It just so happens that in cosmological terms that point is very close to the present time and so the two are close to equal.
In the below graph from Wikipedia, you can see that the start of the curves representing $\Omega_M = 0$ (the Milne model, where the age of the Universe is the inverse of the Hubble constant) and $\Omega_M = 0.3, \Omega_{\Lambda} = 0.7$ (a standard cosmological constant model of dark energy) very nearly coincide.